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Cassini Closing In On Saturn

Cassini Positional chart generated using David Seal's Solar System Simulator at JPL
Pasadena - Mar 12, 2003
The most recent spacecraft telemetry was acquired from the Goldstone tracking station on Wednesday, March 5. The Cassini spacecraft is in an excellent state of health and is operating normally. Information on the present position and speed of the Cassini spacecraft may be found on the "Present Position" web page.

Attitude Control Subsystem (ACS) Flight Software (FSW) checkout continued this week with the following activities uplinked and executed: calibration of inertial reference unit-A, a 7COAST demonstration with rates, star ID suspend demo with rates, checkout of sun sensor assembly-B, several high water mark clears, and fault protection log pointer resets.

Playback data from off-track activities has been received. Everything looks normal, and detailed analysis continues. An inertial reference unit-B checkout and calibration activity was also uplinked for execution next week.

The project held a final uplink approval meeting for the Command and Data Subsystem (CDS) flight software checkout activities. Procedures and files for the checkout were approved, with uplink and checkout activities to begin on March 24.

Preliminary port three for Science Operations Plan implementation of tour sequences S15/S16 occurred this week. The third and final input port occurs next week. Additionally, all teams have been reviewing the first official merged sequence for S17/S18.

The Science Planning Team process for C37 concluded this week with the delivery of the port two products and the handoff package to the Sequence team. Subsequence generation for C37 began with a kick-off meeting held on Tuesday.

The March Instrument Operations working group meeting featured a SEQ_CONVERT tool tutorial by the Mission Sequence Subsystem development team.

System Engineering has created a web page to assist with tour Verification and Validation activities. The site will contain links to various matrices, templates, and documentation in support of V&V. Also posted will be materials presented at last week's Cassini Design Team meeting including a detailed uplink system V&V schedule, and the uplink V&V kickoff agenda.

Delivery coordination meetings (DCM) were held for Version 9 of the Mission Sequence Subsystem, and the Instrument Operations Science Operations and Planning Computer (SOPC) Broadcast Keep-Alive scripts. A number of the keep-alive utilities have been updated due to changes in the Deep Space Mission Services firewall.

The Jupiter Magnetosphere Synchrotron Radiation experiment was noted in the February 2003 "APS News," a publication of the American Physics Society, as a significant Astrophysics event of 2002. Even though the Cassini RADAR is not mentioned by name, it was the radiometer instrument that collected the raw data for the experiment.

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No Rest On The Way To Titan

artwork by David Seal
Paris - Sept 2, 2002
After an adventurous 7-year long tour among the planets, the Cassini-Huygens spacecraft will arrive at Saturn in July 2004. Once there, Cassini will parachute the Huygens probe to Saturn's biggest satellite, Titan. Titan is thought to have an atmosphere similar to the primitive Earth. However, both the probe and the Cassini-Huygens team are not in idle state until 2004. They have plenty of things to keep them busy. Full Details

Rising Storms Revise Story Of Jupiter's Stripes
San Antonio - Mar 07, 2003
Pictures of Jupiter, taken by a NASA spacecraft on its way to Saturn, are flipping at least one long-standing notion about Jupiter upside down.



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